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Teagan Clarke

@astroteagan.bsky.social
1.9K followers 501 following 20 posts

Postdoc | gravitational-wave astronomer | Princeton University | 💫 🏳️‍🌈 🇦🇺

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Reposted by Teagan Clarke
LIGO Scientific Collaboration @ligo.org · 14/09/2026
Happy birthday #GW150914! 11 years ago today, we caught our first gravitational wave, and founded a new type of astronomy A decade later, we now have hundreds of observations! 🔭🧪🎂
Classic plot showing GW150914. Filtered data from LIGO Livingston and LIGO Hanford are shown, both show the characteristic signal of a binary black hole. Crucially, data from the two observatories agree, indicating a real signal.
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Dr Shanika Galaudage @astronerdika.bsky.social · 17/08/2026
It's #NeutronStarWeek! Come with me on a tour through the Universe to meet some iconic neutron stars: pulsars, magnetars, mergers & more! But let's start 130,000,000 light-years away, with two neutron stars that are no more... 👀 #Astronomy #NeutronStars
Infographic, created by Shanika Galaudage, introducing a tour of iconic neutron stars. Large white text reads, “Meet some iconic Neutron Stars:” with orange handwritten text below reading, “pulsars, magnetars & mergers across the Universe!” A pale-blue neutron star with looping magnetic-field lines and a curved dotted beam appears at lower right. The background is a map of the Universe, with faint dashed, logarithmically spaced distance contours labelled in light-years.
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Dr. Sharan Banagiri (he/him) @geodesicvoyager.bsky.social · 06/07/2026
Read about how recent work, including by yours truly, is revealing hierarchical mergers and evidence for multiple subpopulations in this lovely APS physics viewpoint article physics.aps.org/articles/v19...
physics.aps.org
Evidence Mounts for Hierarchical Black Hole Mergers
Different analyses of gravitational-wave observations are converging on evidence for a distinct population of massive black hole binaries produced through repeated mergers.
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Royal Astronomical Society @royalastrosoc.bsky.social · 26/06/2026
We're delighted to announce that Dr Isobel Romero-Shaw has won the 2026 Caroline Herschel Prize Lectureship. Her lecture, at the University of Bath in November, is titled 'Violent Beginnings Have Violent Ends: Deciphering the Origins of Binary Compact Object Collisions with Gravitational Waves'. ⤵️
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Matt Herdman @mattherdman.bsky.social · 01/06/2026
Happy Pride month to the whole LGBTQNJ+ rainbow!
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Nihar Gupte @nihar-gupte.bsky.social · 29/04/2026
Hi everyone I wanted to show a couple features of my website. Firstly, a page which shows evolutions of the binary black holes we have detected with @ligo.org @egovirgo.bsky.social @kagra. Click the link to learn more! nihargupte.com/blog/catalog... #blackholes
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American Astronomical Society (AAS) @aas.org · 03/04/2026
The President's Budget Request proposes a 47% cut to NASA Science, a 55% cut to NSF, and a 13% cut to the DOE Office of Science. AAS President Dr. Dara Norman sent a call to action to AAS members via email today. Urge your members of Congress to reject these cuts now! aas.org/reject-2027-...
Graphic with the text "Action Alert: AAS urges advocacy against proposed cuts to science in President's Budget Request"
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Teagan Clarke @astroteagan.bsky.social · 26/03/2026
very cool astrobite article for a new paper I'm involved with led by Mor Rozner 🧪🔭😎
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EGO and the Virgo Collaboration @egovirgo.bsky.social · 16/03/2026
Last week over 400 scientists of the @ligo.org - Virgo - KAGRA Collaboration met in Pisa, Italy for the LVK Meeting, the biannual gathering of the global community studying gravitational waves 🌟🌍
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Teagan Clarke @astroteagan.bsky.social · 14/12/2025
Snowy Princeton 😍❄️☃️
Princeton's Blair hall pictured on a sunny day covered in snow. A snowman can be seen at the base of the hall A snowy scene of Princeton campus framed by trees. The central building features a white flag with the orange and black Princeton crest  inside A snowy photo of one of the old halls at Princeton University A snowy scene showing Nassau hall at Princeton University with people gathered in the foreground
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LIGO Scientific Collaboration @ligo.org · 18/11/2025
Our fourth LIGO @egovirgo.bsky.social KAGRA observing run has now drawn to a close. We will be busy analysing data for a while to come—watch out for more discovery announcements. We will be back next year observing.docs.ligo.org/plan/
observing.docs.ligo.org
IGWN | Observing Plans
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Dr Shanika Galaudage @astronerdika.bsky.social · 26/09/2025
Mirror, mirror, reflecting our [LASER] beam... What is the loudest [gravitational wave] signal that we've seen? It’s #GW250114! (Yes, it’s been two weeks since it was announced, but I can still celebrate! 🎉 ) #EinsteinWasRight #HawkingWasRight @ligo.org @egovirgo.bsky.social
An infographic created by @astronerdika titled “MIRROR, MIRROR, reflecting our LASER beam… what’s the LOUDEST signal gravitational wave we’ve seen?” explaining the gravitational-wave discovery GW250114 and how the observation confirms Hawking’s area law. The visual shows the mirrors in a gravitational-wave interferometer speaking about the loudest event they have seen. There are several illustrations as follows:

1. A simplified diagram of a laser interferometer. A red laser beam from a labeled “LASER source” hits a beam splitter, travels down two perpendicular arms, reflects off round mirrors, and recombines at a labeled “detector.” A label near the top-right mirror reads: “the DETECTOR, signal seen by LIGO Hanford & LIGO Livingston.”

2. An illustration of a binary black hole merger, with two black circles spiraling inward. They are labeled ~34 solar masses and ~32 solar masses. Surrounding spiral lines represent gravitational waves. A nearby caption reads: “the SOURCE, Discovered in 2025, on January 14, at 08:22:03 UTC.”

3. A prominent speech bubble with white text on a purple background states: “GW250114 is the loudest & clearest signal we’ve seen!” A smaller note below reads: “as of January 2025.”

4. Another speech bubble reads: “AND we saw that Hawking was right too!”

5. Visual explanation of Hawking’s Area Law. Two small circles labeled “this BH” + “this BH” are shown to the left of a “<” symbol, pointing to a larger circle labeled “the surface area of the merged BH.” Below there is the explanatory sentence: “GW250114’s remnant event horizon area is larger than the sum of the individual areas.”

6. A section titled “the PAPERS” lists two arXiv references: https://arxiv.org/abs/2509.08054 and https://www.arxiv.org/abs/2509.08099

Note: This infographic plays off the classic line from Snow White, “Mirror, mirror on the wall…” Here, the “mirrors” are the ones inside the laser interferometer, reflecting light to detect passing gravitational waves.
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Teagan Clarke @astroteagan.bsky.social · 30/08/2025
Occupation: Student'nt Thanks @pinkastrophysicist.bsky.social for making me the delicious cake and taking this photo of me being equally excited and terrified 5 minutes after submitting my PhD 🥰🎂🧑‍🎓
A photo of me in a green vest holding a pink cake with yellow sprinkles that says "p h done". I have a big smile with a slightly anxious look in my eyes
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Monash Astrophysics @monashastro.bsky.social · 29/08/2025
Front page news! 📰 Monash PhD researcher Christian Adamcwicz leads new LVK results revealing the mysterious 40 M☉ gap in black hole populations. Exciting clues about how the universe’s heaviest stars live and die! #BlackHoles #LVK #Astrophysics www.theaustralian.com.au/science/grav...
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LIGO Scientific Collaboration @ligo.org · 26/08/2025
Results from the first part of our fourth LIGO @egovirgo.bsky.social KAGRA observing run are out today! We're pleased to share the largest catalog of gravitational-wave observations with more discoveries of black holes and neutron stars 📰 arxiv.org/abs/2508.18082 🔭🧪⚛️☄️ #GWTC4
New masses in the stellar graveyard plot, showing astronomical observations of black holes and neutron stars. The number of gravitational-wave observations of black holes is overwhelming. The plot is arranged to look nice, the horizontal axis has no meaning, but the vertical one shows masses. We have a significant range of masses from about 1 solar mass to over 200 solar masses for our largest merger remnant. New out today is a neutron star black hole binary GW230518_125908, as well as a lot of binary black holes.
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Teagan Clarke @astroteagan.bsky.social · 26/08/2025
Congrats to everyone in the LVK collaboration who worked so hard to get these exciting results out 🤩🧪🔭
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Teagan Clarke @astroteagan.bsky.social · 01/07/2025
JWST slays with this bisexual lighting for the super fascinating bullet cluster 😍🌈
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NSF–DOE Rubin Observatory @rubinobservatory.org · 22/06/2025
Welcome to a new era in astronomy and astrophysics ✨🔭🧪 Get ready to join us virtually for the reveal of Rubin's first images! #RubinFirstLook 🗓️ June 23, 2025 ⌚️ 11am US EDT 🔗 ls.st/rubin-first-look-livestream
ls.st
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LIGO Scientific Collaboration @ligo.org · 11/06/2025
The gang are all here! Today we resumed our fourth observing run with LIGO Hanford, LIGO Livingston, Virgo, KAGRA and GEO all observing together! You can check detector status live at online.ligo.org ☄️🔭🧪
Detector dashboard showing all five detectors happily in Observing status
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Dr. Skylar Grayson @skylargrayson.bsky.social · 15/04/2025
Did you know NASA science is facing a 50% budget cut??? Please read this @astrobites.bsky.social post to learn more about it and what you can do astrobites.org/2025/04/15/h...
astrobites.org
NASA Needs Your Help!
NASA is facing severe budget cuts that would cancel missions ready to be launched, put tens of thousands out of a job, and set science back decades. We need your help to ask congress to prevent these ...
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Teagan Clarke @astroteagan.bsky.social · 16/04/2025
Publication day! With @sarinastro.bsky.social , Eric Howell, @plasky.bsky.social and Eric Thrane, we explore a hypothetical coincident neutron star-black hole merger and fast radio burst. We hope this work helps pave the way for future multimessenger detections! 🔭🧪⚛️ journals.aps.org/prd/abstract...
journals.aps.org
Quantifying the coincidence between gravitational waves and fast radio bursts from neutron star-black hole mergers
Fast radio bursts (FRBs) are mysterious astrophysical transients whose origin and mechanism remain unclear. Compact object mergers may be a promising channel to produce some FRBs. Neutron star--black ...
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MPI for Multidisciplinary Sciences @mpi-nat.bsky.social · 11/04/2025
Live from the kestrel box: Season 2 is now streaming! Our kestrel camera is back online – the first eggs have arrived. 🥚🥚 Drop by our kestrel couple 🦅 and watch the little family grow. www.mpinat.mpg.de/kestrel-camera #MPI_BioDiversum #KestrelCamera #LiveStream #Kestrels
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Emily Hunt @emily.space · 12/03/2025
Oh wow, this is *such* a cool concept - a 'game' procedurally generated from Wikipedia, in which you can literally traverse all of human knowledge and walk down rabbit holes
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Martha Rich Art Projects @martharichart.bsky.social · 27/02/2025
I made this the other night while procrastinating, mainly because I thought all the posts about the blackout were boring. It feels like there is momentum bringing people together!
A poster for the economic blackout on February 28. It is a big red Jack rabbit on an aqua blue back ground. It says economic blackout in hand done black type. There are two black speech bubbles. One says “don’t buy stuff Friday February 28th. The other says we have power. Below it says No Amazon, Walmart, target, gas food, gas. Below that it says OK small business, use cash. Designed by Martha Rich.
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Emily Hunt @emily.space · 17/02/2025
The best dark sky in the world - the Atacama Desert in Chile, which hosts many @eso.org telescopes - is under threat from an industrial project. 🔭 Astronomers can sign a petition in favour of moving the planned industrial project: docs.google.com/forms/d/e/1F...
eso.org
World's darkest and clearest skies at risk from industrial megaproject
On December 24th, AES Andes, a subsidiary of the US power company AES Corporation, submitted a project for a massive industrial complex for environmental impact assessment. This complex threatens the pristine skies above ESO’s Paranal Observatory in Chile’s Atacama Desert, the darkest and clearest of any astronomical observatory in the world [1]. The industrial megaproject is planned to be located just 5 to 11 kilometres from telescopes at Paranal, which would cause irreparable damage to astronomical observations, in particular due to light pollution emitted throughout the project’s operational life. Relocating the complex would save one of Earth's last truly pristine dark skies.
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LIGO Scientific Collaboration @ligo.org · 11/02/2025
#February11 is the International Day of Women and Girls in Science #IDWGS. Meet some of our international #WomenInSTEM through #HumansOfLIGO 1/🧵
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Point Defiance Zoo & Aquarium @ptdefiancezoo.bsky.social · 04/02/2025
Exciting news! We’re thrilled to announce that tapir Yuna gave birth to a rare and endangered Malayan tapir calf Sunday night. The newborn, covered in distinctive white spots and stripes resembling a fuzzy walking watermelon, is only the second tapir born in our 120-year history.
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Alastair Williams @alastairwilliams.bsky.social · 03/02/2025
ESO has some fantastic images of comet C/2024 G3 from their observatory in Chile 🧪🔭 Credit for this one belongs to F. Millour/ESO
A bright comet seen next to the telescopes of the ESO observatory in Chile
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CosmicRami 🏳️‍🌈🏳️‍⚧️ @rami.spaceaustralia.com · 30/01/2025
The most shocking part of this photo are the words that have not been painted over as yet. They aren't even all "DEI" words. And yet, they are being wiped away. A re-write of history's lessons, the removal of the things that build a functioning society, to please the Emperor.
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Max-Planck-Gesellschaft @maxplanck.de · 28/01/2025
Here is a highly recommended thread that summarizes what has happened in scientific landscape in the US since Trump's inauguration. It makes for dystopian reading ⬇️
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Ayana Elizabeth Johnson @ayanaeliza.bsky.social · 24/01/2025
As expected, the Trump team is already deleting climate info from government websites. In anticipation, our team at Urban Ocean Lab created a permanent archive of 100+ key resources and published a permanent archive: www.urbanoceanlab.org/resource-hub 👩🏽‍💻
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Katie Mack @astrokatie.com · 22/01/2025
Petro, in 2021: “At NASA and Kennedy Space Center, our commitment to diversity, equity, inclusion and accessibility has been paramount to mission success.”
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Teagan Clarke @astroteagan.bsky.social · 23/01/2025
NASA working fast to remove any trace of EDI from their website... www.nasa.gov/odeo/diversi...
nasa.gov
Diversity & Inclusion - NASA
A diverse and inclusive workforce fueled by innovation and united in achieving mission success for NASA.
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Emily Hunt @emily.space · 17/01/2025
we have a pypi pypi.org/project/SK8p...
pypi.org
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Teagan Clarke @astroteagan.bsky.social · 12/01/2025
Link to a Disaster Relief fund to help the 200+ Caltech Community Members - including several LIGO collaboration members - who have lost their homes to the fires: giving.caltech.edu/areas-to-sup... please share and / or donate if you can!
giving.caltech.edu
The Caltech and JPL Disaster Relief Fund
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Marcus Lower @astromelow.bsky.social · 07/01/2025
I am looking to hire a PhD student at Swinburne University to study the links between pulsars, magnetars and fast radio bursts! If you or anyone you know may be interested, then please feel free to reach out to me via email. #Astronomy #RadioAstronomy astronomy.swin.edu.au/study/phdpro...
Artists impression of a magnetar: a compact spherical star surrounded by twisted magnetic field lines and glowing plasma.
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CosmicRami 🏳️‍🌈🏳️‍⚧️ @rami.spaceaustralia.com · 06/01/2025
The Earth-based gravitational wave detectors (LIGO/VIRGO/KAGRA) looked for continuous GWs across 45 pulsars (which can be formed by tiny little mountains on their surface) but found no continuous GWs. Sadness. [note - these are not the GWs we search for in pulsar timing] arxiv.org/abs/2501.01495
arxiv.org
Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run
Continuous gravitational waves (CWs) emission from neutron stars carries information about their internal structure and equation of state, and it can provide tests of General Relativity. We present a ...
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Anna Hughes 🍁 @annaghughes.bsky.social · 22/12/2024
Think twice before gifting someone an M dwarf this holiday season
An M dwarf star with the text: "I am not a toy. I am not a Christmas present. I am a 10 trillion year commitment"
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Bluesky @bsky.app · 03/12/2024
Scientists, academics, researchers: We’re excited to share that @altmetric.com is now tracking mentions of your research on Bluesky! 🧪
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Teagan Clarke @astroteagan.bsky.social · 03/12/2024
Hot off the press paper co-lead by @pinkastrophysicist.bsky.social - mapping the gravitational wave background across the sky 🤩🔭🧪⚛️
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Rowina Nathan ✨ @pinkastrophysicist.bsky.social · 02/12/2024
What generates the gravitational waves that make up the background? It is probably supermassive black-hole binaries and/or early Universe physics. We don't know yet but it is likely a combination of both! 💥 It's paper release day tomorrow! Excited to share with you all!
A graphic comparing gravitational wave background sources. The left shows a black hole binary and the right shows some bubbles. The text on the left reads "SUPERMASSIVE BLACK
HOLE BINARIES
Extraordinarily massive black holes in the center of galaxies orbiting eachother,
GW Signal: Anisotropic Different in different directions
Allows us to study: Galaxy formation, mass distribution of Universe, gravity"
The text on the right reads "PRIMORDIAL UNIVERSE
PHYSICS
Colisions between 'bubbles' in the hot, dense, 'boiling' early Universe soup
*+ GW Signal: Isotropic - Same in all directions
Allows us to study: The Big Bang, early
Universe, particle physics"
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Natasha Van Bemmel @natasha-vb.bsky.social · 26/11/2024
My first first-author paper just dropped on arXiv ✨👩‍🔬🧪🔭 Introducing the KiloNova and Transients Program (KNTraP), a search specifically designed to find a kilonova. Check it out here to see the methods developed to scour the data for kilonova candidates, and what we found: arxiv.org/abs/2411.16136
Abstract of the KNTraP paper.

Text: Compact binary mergers detectable in gravitational waves can be accompanied by a kilonova, an electromagnetic transient powered by radioactive decay of newly synthesised r-process elements. A few kilonova candidates have been observed during short gamma-ray burst follow-up, and one found associated with a gravitational wave detection, GW170817. However, robust kilonova candidates are yet to be found in un-triggered, wide-field optical surveys, that is, a search not requiring an initial gravitational wave or gamma-ray burst trigger. Here we present the first observing run for the Kilonova and Transients Program (KNTraP) using the Dark Energy Camera. The first KNTraP run ran for 11 nights, covering 31 fields at a nightly cadence in two filters. The program can detect transients beyond the LIGO/Virgo/KAGRA horizon, be agnostic to the merger orientation, avoid the Sun and/or Galactic plane, and produces high cadence multi-wavelength light curves. The data were processed nightly in real-time for rapid identification of transient candidates, allowing for follow-up of interesting candidates before they faded away. Three fast-rising candidates were identified in real-time, however none had the characteristics of the kilonova AT2017gfo associated with GW170817 or with the expected evolution for kilonovae from our fade-rate models. After the run, the data were reprocessed, then subjected to stringent filtering and model fitting to search for kilonovae offline. Multiple KNTraP runs (3+) are expected to detect kilonovae via this optical-only search method. No kilonovae were detected in this first KNTraP run using our selection criteria, constraining the KN rate to R<1.8×10^5 Gpc−3 yr−1.Plot showing the volume per night covered by a survey. Volume increases towards the top right corner of the plot. DES survey is shown leftmost, then further right is KNTraP with multiple volumes demonstrating the balance between of number of fields/area on sky observed per night versus the depth achieved, both in dark and bright sky time. Rightmost shown are projected KWFI nightly volumes.
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Teagan Clarke @astroteagan.bsky.social · 26/11/2024
Opportunity to join the astronomy group at Monash and live in the best Australian city- Naarm/Melbourne 🤩 ☕
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Rowina Nathan ✨ @pinkastrophysicist.bsky.social · 25/11/2024
What is the difference between gravitational-wave signals measured by LIGO and pulsar timing arrays? Well lots of things, but mainly the mass of the black holes. This infographic summarises the differences. 👀🕳️💫
An infographic explaining different black hole mergers. The left side shows two smaller black holes spiralling inwards. The right shows two larger black holes orbiting each other. The text on the left reads: "BINARY BLACK HOLE
MERGER
Observed by: ground-based detectors.
Detector lenth: kilometers
Solar masses: tens to hundreds
Found in: everywhere?
Merger time: seconds
GW period: milliseconds
"Sounds like':) chirp, bang, crash"
The text on the right reads: "SUPERMASSIVE
BINARY BLACK HOLE
Observed by: putsar timing arrays
Detector length: kiloparsecs
Solar masses: millions to billions
Found in? center of large galaxies
Merger time: millions of years*
GW period: years
'Sounds like': rumble, hum"
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Kanaya Malakar @kanaya-malakar.bsky.social · 21/11/2024
I had a hard time finding women physicists here. So I made a starter pack for #female and #under-represended #minorities in #physics, in short #FURMIP. Please spread the word and let me know if you would like to be added. go.bsky.app/2JeYsDz
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Dr Shanika Galaudage @astronerdika.bsky.social · 21/11/2024
Well ain’t this just… WICKED! 💚🩷 It’s amazing to see the growth in the number of folks with qualifications #physics and #astronomy in Oz 🇦🇺✨
An infographic with a bar chart that looks like towers showing the growth in the population of folks with a qualification in physics and astronomy in Australia.
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Sesh Nadathur @seshnadathur.bsky.social · 20/11/2024
Big paper day today! 🔭🧪 The newest results from the Dark Energy Spectroscopic Instrument or DESI newscenter.lbl.gov/2024/11/19/n... 8 new papers on the arXiv this morning, including the long awaited analysis of the "full shape" of the galaxy power spectrum, and one led by my PhD student.
newscenter.lbl.gov
New DESI Results Weigh In On Gravity
Researchers used the Dark Energy Spectroscopic Instrument to map how nearly 6 million galaxies cluster across 11 billion years of cosmic history. Their observations line up with what Einstein's theory...
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Leo C. Stein @duetosymmetry.com · 20/11/2024
❤️ ❤️ Black hole binary 💕 Compact binary 💞 Late inspiral, merger 💓 Ringdown ❤️ Remnant 🧪⚛️🔭
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Paarmita Pandey @astrofermi.bsky.social · 19/11/2024
It's PAPER DAY 📣 My first first-author paper is now published in ApJ 🎉 Read about how star clusters contribute as galactic cosmic ray sources. Comments and questions are welcome 🤗 Gamma-Ray Emission from the Star-forming Region RCW 38 iopscience.iop.org/article/10.3...
iopscience.iop.org
Constraining the Diffusion Coefficient and Cosmic-Ray Acceleration Efficiency Using Gamma-Ray Emission from the Star-forming Region RCW 38 - IOPscienceSearchopens in new tab
Constraining the Diffusion Coefficient and Cosmic-Ray Acceleration Efficiency Using Gamma-Ray Emission from the Star-forming Region RCW 38, Paarmita Pandey, Laura A. Lopez, Anna L. Rosen, Todd A. Thom...
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Christopher Berry @cplberry.bsky.social · 19/11/2024
To accompany all those BlueSky science/academia #starterpacks, let’s share introductions to the literature of our fields Gravitational-wave papers (created with observablehq.com/@guillaume-l...) When the intro starts "We have opened a new window" you know you can skip a couple of paragraphs
Most scientific papers in xkcd comic style, with titles:

We did. We detected gravitational waves!

2000 people worked for 3 years on this and you're just going to read Section D5 and look at plots

We calculated these pN equations so you don't have to 

Binaries stars: Even more complicated

We know you're tired of citing Abbott et al. Here's an Abac et al

This will be great if we build it in 2050

We thought of a new way Einstein could be wrong. The data say he isn't. Yet

Upper limits are neat: We looked really hard and still haven't found anything

We hid the quantum uncertainty down the back of the sofa and improved detector performance

Something exploded and we all saw it! Isn't multi messenger astronomy fun (paper 1 of 49)

Some thoughts on what even is a black hole really?

Glitches: caused by dark magic?
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